Dear Colleagues, It looks that some worked targets will be done soon, with only one or two more sessions. Others are no longer reachable for some of you, or critical phases in them don't occur during your observing windows. So, it has come a time to provide you a new list of targets. Before you start a new target from the list in section 5 below, please first check whether you cannot contribute to some of the higher priority targets in sections 0 to 2 (also don't forget to check their status in the binast-webtool). Enjoy. This list of targets is also available on http://www.asu.cas.cz/~asteroid/binastphotsurvey_listoftargets20090402.txt Clear Skies, Petr Pravec Object V Dec Elo Mot Bga H q a Arc Hrev P Ampl U 0. Worked objects: (1344) Caubeta 15.0 11 159v 0.2 68 12.8 1.98 2.25 21opp More data needed, currently under control by Don. (1676) Kariba 14.6 0 170^ 0.3 62 12.7 1.82 2.24 19opp One long session might nail it down. (2577) Litva 15.7 3 120v 0.4 27 13.2 1.64 1.90 15opp Binary, one good long session for each of the two events is needed to nail down the solution, see events ephemeris on the binast-webtool. (3309) Brorfelde 16.7 42 118v 0.4 49 13.9 1.72 1.82 10opp Return binary, one additional long session (at any orbital phase) needed to nail down solution. (4607) Seilandfarm 16.3 8 138v 0.1 46 12.9 2.22 2.26 13opp Binary, one good long session covering the secondary event may suffice to nail down its D2/D1. (7033) 1994 WN2 16.5 17 139v 0.1 54 13.3 2.14 2.24 10opp More data needed (two attenuations observed so far) (7557) 1982 FK3 16.4 5 152v 0.1 55 13.8 1.92 2.47 12opp Under control by Don. (11116) 1996 EK 16.0 14 148v 0.2 62 14.1 1.70 2.20 12opp More data with errors 0.01 mag needed to establish this probable binary. (139537) 2001 QE25 17.7 -4 178v 0.3 58 14.9 1.93 2.68 6opp Paired asteroid, longer period, linked data needed. Object V Dec Elo Mot Bga H q a Arc 1. Returning binaries (175706) 1996 FG3 15.9 -12 168v 1.1 49 18.2 0.69 1.05 7opp NEA binary, observations needed to refine its orbital solution as well as to support planned observations on other wavelengths. 2. Returning "prime suspects", to be followed up on their 2nd (3rd, ...) apparitions (2648) Owa 16.4 -16 167^ 0.3 46 12.9 1.86 2.25 10opp 12.9 3.5641 0.23 3 (3913) Chemin 14.6 20 136 0.4 56 12.2 1.83 2.36 9opp 12.2 3.4077 0.17 3- 3. Paired asteroids (errors <0.05 mag needed): 4. YORP detection target: 5. New targets (3825) Nurnberg 15.1 0 169^ 0.2 62 13.0 2.03 2.24 19opp (4171) Carrasco 15.0 -7 171^ 0.3 56 12.9 2.07 2.24 11opp (4594) Dashkova 16.0 -2 174^ 0.3 61 14.3 1.88 2.19 13opp (4795) Kihara 16.2 -3 159^ 0.2 54 13.9 1.86 2.20 11opp (5752) 1992 CJ 15.4 -9 173^ 0.3 54 13.4 1.97 2.24 13opp (6319) Beregovoj 16.0 -7 173^ 0.3 55 13.9 2.08 2.27 11opp (20634) Marichardson 16.2 2 172 0.2 65 14.0 2.10 2.45 10opp (37601) Vicjen 15.8 25 149 0.5 84 14.1 1.72 2.26 7opp (39810) 1997 WQ35 15.5 43 132 0.3 74 13.6 1.68 2.31 9opp (93768) 2000 WN22 15.3 17 133^ 0.2 51 13.7 1.59 2.33 6opp (132124) 2002 CW237 16.1 32 141 0.5 76 14.4 1.64 2.34 4opp Note: The ephemerides were computed for 2009-04-02 ^/v means that the value increases/decreases by more than 0.05 mag/day (for V) or by more than 0.5 deg/day for Dec and Elong. The rate of apparent motion (Mot) is in deg/day. Bga is the galactic latitude. Compact listing: (1344) (1676) (2577) (3309) (4607) (7033) (7557) (11116) (139537) (175706) (2648) (3913) (3825) (4171) (4594) (4795) (5752) (6319) (20634) (37601) (39810) (93768) (132124)